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Integrity report for The evolution of magnetic hot massive stars: Implementation of the quantitative influence of surface magnetic fields in modern models of stellar evolution

A machine-verified record of the checks Pith has run against this paper: detector runs, findings, signed bundle events, and canonical identifiers.

arXiv:1702.04460 · pith:2017:MCVBC3PM6WGLIK3QSL4CXWB7EJ

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Paper page arXiv integrity.json bundle.json

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Signed record

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